Matter of subnuclear density in the inner crusts of neutron stars consists of neutron-rich atomic nuclei immersed in strongly degenerate relativistic gas of electrons and strongly nonideal liquid of neutrons. Thermodynamic and kinetic properties of this matter are greatly affected by Coulomb and nuc
Nuclear structure and dynamics in the inner crust of neutron stars
β Scribed by P. Magierski; A. Bulgac
- Publisher
- Elsevier Science
- Year
- 2004
- Tongue
- English
- Weight
- 377 KB
- Volume
- 738
- Category
- Article
- ISSN
- 0375-9474
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π SIMILAR VOLUMES
We perform a detailed calculation of the pairing properties of the inner crust of a neutron star. We focus on a specific density, and take into account the coexistence of a nuclear lattice with a superfluid gas of neutrons. The Hartree-Fock-Bogoliubov (HFB) equations are solved adding the matrix el
We present a novel method to study the dynamics of bulk fermion systems such as the neutron star's crust. By introducing periodic boundary conditions into Fermionic Molecular Dynamics, it becomes possible to examine the long-range many-body correlations induced by antisymmetrisation in bulk fermion